Physics
Scientific paper
Mar 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1286s&link_type=abstract
43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1286
Physics
Scientific paper
The SW-Fe suggests an additional source of npFe0 in the lunar regolith.
This source can be important, since much more volatile helium-3, having
lower SW-concentartion than SW-Fe, is nevertheless detected in the lunar
regolith and suggested as a fuel.
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